Mathematical tracts on the lunar and planetary theories, the figure of the earth, precession and nutation, the calculus of variations, and the undulatory theory of optics.

80 PLANETARY TIIEORY. value only commensurate with their value in r$r, and consequently, though considerable, they cannot rise to first-rate importance. We shall therefore confine our attention to the term depending on cos (pnt - qn't + Q) where pn - qn' is very small. The period of the force which produces this 27r terni is n-, and is therefore very great. The period pn - qn of the inequality is the same. It appears then that the terms which l)ecome very great are those which occupy a very long period, and which in consequence can hardly be discovered from observations that extend through a short time. Thus the inequality of Saturn produced by Jupiter (and a corresponding one of Jupiter) depending on cos5(nt + ) -2(n't + ) + Q, has a period exceeding 900 years, or 30 revolutions of the exterior planet. The inequality of the Earth alluded to in (94) las a period of about 240 years, or 240 revolutions of the exterior planet. There are many similar terms in the theory of the different planets, but no others so remarkable as these. 101. The increase of the coefficient from integration is inversely as (p z - qn')2, or directly as ( ----, or directly \pBn-q/n as thi square of the period of the inequality. Of this, the following popular explanation may be offered. If we conceive a force to urge the planet in the same direction for a long time, or if we conceive the preponderance of forces acting in one direction over those acting in the opposite direction to be of the same kind for a long time, (which may be the case when pn - qn' is small, because then the periodic times of the two planets are in the proportion of p: q very nearly, and therefore after q revolutions of one planet or p revolutions of the other, they will again be in nearly the saine relative situation at the same parts of their orbits, and thus the actions of the same kind are repeated over and over again for a long time), the velocity of the planet may be increased so that it describes a larger orbit than before, and its periodic time will therefore be increased,

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Title
Mathematical tracts on the lunar and planetary theories, the figure of the earth, precession and nutation, the calculus of variations, and the undulatory theory of optics.
Author
Airy, George Biddell, Sir, 1801-1892.
Canvas
Page 68
Publication
Cambridge,: J. & J.J. Deighton;
1842.
Subject terms
Celestial mechanics.
Calculus of variations
Geometrical optics.

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"Mathematical tracts on the lunar and planetary theories, the figure of the earth, precession and nutation, the calculus of variations, and the undulatory theory of optics." In the digital collection University of Michigan Historical Math Collection. https://name.umdl.umich.edu/aan8938.0001.001. University of Michigan Library Digital Collections. Accessed May 1, 2025.
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